This topic investigates the 'fire-born' rocks, focusing on the journey from molten magma to solid crystalline structures. Students explore how the environment of cooling, whether deep underground or on the surface, dictates the texture and grain size of the resulting rock. This is a fundamental part of the OCR Geology specification, requiring students to classify rocks like granite, basalt, and gabbro based on their mineralogy and cooling history.
National Curriculum Attainment TargetsOCR Geology AS/A-level: 2.2.1 Magma generationOCR Geology AS/A-level: 2.2.2 Igneous rock classification
Using salol (phenyl salicylate) on warm and cold microscope slides, students observe crystal growth in real-time. They record how the speed of cooling directly impacts the size of the crystals formed, mimicking intrusive and extrusive environments.
How does cooling rate affect the texture of igneous rocks?
Groups are given cards representing different minerals. They must arrange them in the order they crystallise from a melt (Bowen's Reaction Series) and then predict which minerals will be found together in mafic vs. felsic rocks.
What is the difference between mafic and felsic magmas?
Display samples showing vesicular, porphyritic, glassy, and phaneritic textures. Students move between stations to sketch the textures and hypothesize the specific volcanic or plutonic events that created them.
How do intrusive and extrusive environments shape rock formation?
Magma is molten rock below the surface; lava is molten rock that has erupted. This distinction is crucial because the presence of volatiles (gases) and the cooling rate differ significantly between the two. Using a 'bottled soda' analogy helps explain the role of pressure and gas release.
All igneous rocks are formed from volcanoes.
The majority of igneous rocks (plutonic) form deep underground and are only seen after millions of years of erosion. Comparing the volume of batholiths to volcanic cones in a visual diagram helps correct this surface-level bias.